This sequence compares Chandra's X-ray image of 3C58 with the views seen by optical and radio telescopes. The intricate X-ray loops in the Chandra image and the features in the radio images of 3C58 extend a dozen light years from the pulsar, likely representing the complex magnetic field structure there.
[Run Time: 0:32](Credit: X-ray: NASA/CXC/SAO/P.Slane et al.; Optical: DSS; Radio: NCSU/S.Reynolds)

In this series of X-ray images, the strong similarities between the center of 3C58 and the Crab Nebula pulsar -- one of the most famous objects in astronomy -- are shown. The 3C58 pulsar, the Crab Nebula pulsar, and a growing list of other pulsars offer dramatic proof that strong electromagnetic fields around rapidly rotating neutron stars are powerful generators of both high-energy particles and magnetic fields.
[Run Time: 0:22](Credit: 3C58: NASA/CXC/SAO/P.Slane et al.; Crab: NASA/CXC/ASU/J.Hester et al.)